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dc.contributor.authorHamilton, Christopher W.
dc.date.accessioned2020-02-14T01:03:20Z
dc.date.available2020-02-14T01:03:20Z
dc.date.issued2020-02-14
dc.identifier.citationHamilton, C. W. (2020) Supplemental information for “Lava-rise plateaus and inflation pits in the McCartys lava flow-field, New Mexico: An analog for pāhoehoe-like lava flows on planetary surfaces”, University of Arizona Campus Repository, https://hdl.handle.net/10150/637043
dc.identifier.urihttp://hdl.handle.net/10150/637043
dc.descriptionThe table “Table_S1.xls” includes the source data used to make Figures 7a, 7b, 7c, 10a, 10b, and 12c in Hamilton et al. (2020), which is an article accepted for publication with Journal of Geophysical Research—Planets. Table S1 is a Microsoft Excel spreadsheet that includes three tabs. The first tab (labeled “Figure_7”) provides strike/dip measurements for the fractures located within the (a) interior, (b) transitional, and (c) steep-sided facies of the lava-rise plateau margin depicted in Figure 7 of Hamilton et al. (2020). Strike and dip values are reported in degrees using the right-hand rule, with strike ranging from 000° to 360° (0°/360° corresponds to North) and dip ranging from 00° to 90° (90° corresponds to vertical) For example, a measurement of 180/60 would correspond to a fracture with a dip (i.e., the slope) that is inclined 60° from horizontal, with dip direction pointing due West (i.e., 270°). The second tab (labeled “Figure_10”) includes two columns of information, containing the locations of all flow indicator used to generate the rose diagrams presented in Figures 10a and 10b, respectively. Locations are specified with X (Easting) and Y (Northing) coordinates, reported in meters within Universal Transverse Mercator (UTM) Zone 13N using the World Geodetic System 1984 (WGS84) datum. Flow directions are reported in degrees, with 0°/360° corresponding to North. The third tab (labeled “Figure_12”) includes the point cloud data used to generate the cross-sectional profile shown in Figure 12c. Each point is specified using X (Easting), Y (Northing), and Z (Elevation) values, which is reported in meters within UTM Zone 13N using WGS84. Digital Number (DN) values provide color information within Red (R), Blue (B), and Green (G) channels, with DN values ranging from 0 to 255. Methods of data production for each of these data sets are described in the Methods Section (§4) of the manuscript. The movie files “Video_S1.mp4” and “Video_S2.mp4” are digital renderings of kite-derived orthomosaic draped over the corresponding digital terrain model (DTM), which is described in §4.1.1 and §5.1 of Hamilton et al. (2020). The renderings were generated using Pix4D software and the source data is available via the University of Arizona Spatial Data Explorer (http://dx.doi.org/10.2458/azu_geo_mccartys_2015).en_US
dc.language.isoenen_US
dc.publisherUniversity of Arizonaen_US
dc.rightsCopyright © 2020 Christopher W. Hamilton. Distributed under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License (CC BY-NC-SA 4.0)en_US
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/4.0/
dc.titleSupplemental information for "Lava-rise plateaus and inflation pits in the McCartys lava flow-field, New Mexico: An analog for pāhoehoe-like lava flows on planetary surfaces"en_US
dc.typeDataseten_US
dc.typeVideo
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizonaen_US
dc.description.noteAcknowledgements:
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en_US
refterms.dateFOA2020-02-14T01:03:25Z


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Copyright © 2020 Christopher W. Hamilton. Distributed under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License (CC BY-NC-SA 4.0)
Except where otherwise noted, this item's license is described as Copyright © 2020 Christopher W. Hamilton. Distributed under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License (CC BY-NC-SA 4.0)